Title: Intermittency in the Photosphere and Corona as Derived from Hinode Data
1Intermittency in the Photosphere and Corona as
Derived from Hinode Data
- Valentina Abramenko
- Vasyl Yurchyshyn
- Big Bear Solar Observatory of NJIT
- Haimin Wang
- CSTR/NJIT
2What is the intermittency look like?
Intermittent Network
Non-intermittent Network
Spatial Domain
Temporal Domain
time
time
3Magnetic field in NOAA10930 from Hinode/SOT/FG
- Extended spatial/temporal intervals of low
activity are intermittent - with compact intervals of enhanced activity.
- Intermittency presents in both spatial and
temporal domains.
4Intermittency can be derived from the Structure
Functions
2D x(x1,x2)
1D x t
r
u(x)
x2
x1
5 Flatness function as an indicator of
intermittency
Structure Functions
Inertial range
Fatness F( r ) is a constant for a
non-intermittent variable and grows as a power
law when scale r vanishes for an intermittent
variable
?
Flatness Function
The intermittency index ?
Scale, r
6NOAA 10930sole on the solar disk
7NOAA 10930intermittency in the corona
Three subsets of Hinode XRT/Be-Thin
area-integrated flux Time Series
Dec 13
Dec 11
Dec 10
8NOAA 10930intermittency in the corona
Three subsets of Hinode XRT/Be-Thin
area-integrated flux Flatness Functions
9NOAA 10930intermittency in the corona
Five subsets of Nobeyama Radioheliograph data
polarization at 9.4 GHz, Time Series
10NOAA 10930intermittency in the corona
Five subsets of Nobeyama Radioheliograph data
polarization at 9.4 GHz, Time Series
11NOAA 10930photospheric intermittency
Hinode SOT/FG magnetogram
To calculate intermittency in the photosphere,
we utilized 2D magnetic field images derived
with Hinode SOT/FG instrument. The covered time
interval 2006 Dec 8/1200 UT to 2006 Dec
13/1845 UT.
Advantages high resolution,
high time cadence,
uninterrupted measurements for several days
12NOAA 10930 intermittency in the photosphere and
corona
13Conclusion
- Highly non-Gaussian, intermittent character of
the magnetic fields in the both photosphere and
corona - The data allow to suggest that intermittency is
preliminary stored in the photosphere and then it
is transported into the chromosphere/corona.
14Conclusions
- The direct connection between the complex
dynamics of the photosphere and corona may be
suggested, and this connection requires a new
kind of linking one associated with the
transfer of information between complex systems.
This standpoint offers new possibilities for the
photosphere / corona coupling.